Suppression of star formation in low-mass galaxies caused by the reionization of their local neighbourhood

Taha Dawoodbhoy, Paul R. Shapiro, Pierre Ocvirk, Dominique Aubert, Nicolas Gillet, Jun Hwan Choi, Ilian T. Iliev, Romain Teyssier, Gustavo Yepes, Stefan Gottlöber, Anson D'Aloisio, Hyunbae Park, Yehuda Hoffman

Research output: Contribution to journalArticlepeer-review

25 Scopus citations

Abstract

Photoheating associated with reionization suppressed star formation in low-mass galaxies. Reionization was inhomogeneous, however, affecting different regions at different times. To establish the causal connection between reionization and suppression, we must take this local variation into account. We analyze the results of CoDa ('Cosmic Dawn') I, the first fully coupled radiation-hydrodynamical simulation of reionization and galaxy formation in the Local Universe, in a volume large enough to model reionization globally but with enough resolving power to follow all atomic-cooling galactic halos in that volume. For every halo identified at a given time, we find the redshift at which the surrounding IGM reionized, along with its instantaneous star formation rate ('SFR') and baryonic gas-to-dark matter ratio (Mgas/MDM). The average SFR per halo with M < 109M was steady in regions not yet reionized, but declined sharply following local reionization. For M > 1010M, this SFR continued through local reionization, increasing with time, instead. For 109M < M < 1010M, the SFR generally increased modestly through reionization, followed by a modest decline. In general, halo SFRs were higher for regions that reionized earlier. A similar pattern was found forMgas/MDM, which declined sharply following local reionization forM < 109M. Local reionization time correlates with local matter overdensity, which determines the local rates of structure formation and ionizing photon consumption. The earliest patches to develop structure and reionize ultimately produced more stars than they needed to finish and maintain their own reionization, exporting their 'surplus' starlight to help reionize regions that developed structure later.

Original languageEnglish (US)
Pages (from-to)1740-1753
Number of pages14
JournalMonthly Notices of the Royal Astronomical Society
Volume480
Issue number2
DOIs
StatePublished - Oct 2018
Externally publishedYes

All Science Journal Classification (ASJC) codes

  • Astronomy and Astrophysics
  • Space and Planetary Science

Keywords

  • Cosmology: theory
  • Dark ages
  • First stars
  • Reionization

Fingerprint

Dive into the research topics of 'Suppression of star formation in low-mass galaxies caused by the reionization of their local neighbourhood'. Together they form a unique fingerprint.

Cite this